G. H. Choi (Author), Y. Amarea (Author), D. Angelaszek (Author), N. Anthony (Author), M. Chung (Author), M. Copley (Author), L. Derome (Author), L. Eraud (Author), C. Falana (Author), J. P. Lundquist (Author)

Abstract

The Cosmic Ray Energetic And Mass for the International Space Station (ISS-CREAM) experiment is designed for precision measurements of energy spectra and elemental composition of cosmic rays. It was launched and installed on the ISS in August 2017. The Silicon Charge Detector (SCD), placed at the top of the ISS-CREAM payload, consists of 4 layers with a total of 10,752 silicon pixels which have 1.37 × 1.57 cm^2 size each. Each layer is arranged in such a fashion that its active detection area of 78 × 74 cm^2 is free of any dead area. The SCD 4-layer configuration was chosen to achieve the best precision in measuring the charge of cosmic rays from proton to iron nuclei with a charge resolution of 0.1 − 0.3e. We will present its on-orbit performance and operation status on the ISS since the launch.

Keywords

instrumentations;high energy cosmic rays;particle detectors;

Data

Language: English
Year of publishing:
Typology: 1.08 - Published Scientific Conference Contribution
Organization: UNG - University of Nova Gorica
UDC: 539.1
COBISS: 50525699 Link will open in a new window
ISSN: 1824-8039
Views: 1636
Downloads: 0
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Other data

URN: URN:SI:UNG
Pages: str. 1-7
Chronology: 2019
ID: 12544189
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